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Solar flares - Magnetohydrodynamic instabilities

open access: yes, 1981
It is pointed out that most solar flares are either simple-loop (or compact) flares or two-ribbon flares. A single loop brightens and decays without moving, whereas the appearance of the two-ribbon type involves the eruption of a magnetic arcade.
Hood, A. W.   +3 more
core   +1 more source

A physics-based method that can predict imminent large solar flares: data and programs

open access: yes
This repository includes all the data (DATA_kappa.tar) and the software (Cal_kappa.tar) to reproduce the results of the paper “A physics-based method that can predict imminent large solar flares” by Kanya Kusano, Tomoya Iju, Yumi Bamba, and Satoshi Inoue.
Kusano, Kanya
core  

Solar and stellar flares and their connection [PDF]

open access: yes
This thesis focuses on bridging the gap between solar and stellar physics through the study of flares. Solar flares are the most powerful explosions in the solar system and many stellar flares have been observed to be orders of magnitudes larger ...
Doyle, Lauren
core  

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